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- W3090335060 abstract "Context. The 6.7 GHz maser transition of methanol has been found exclusively towards massive star forming regions. A majority of the masers have been found to lack the presence of any associated radio continuum. This could be due to the maser emission originating prior to the formation of an H ii region around the central star, or from the central object being too cool to produce a H ii region. Aims. One way to distinguish between the two scenarios is to determine and model the spectral energy distributions (SEDs) of the masers. Methods. We observed a sample of 20 6.7 GHz methanol masers selected from the blind Arecibo survey, from centimeter to submillimeter wavelengths. We combined our observations with existing data from various Galactic plane surveys to determine SEDs from centimeter to near-infrared wavelengths. Results. We find that 70% of the masers do not have any associated radio continuum, with the rest of the sources being associated with hypercompact and ultracompact H ii regions. Modeling the SEDs shows them to be consistent with rapidly accreting massive" @default.
- W3090335060 created "2020-10-08" @default.
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- W3090335060 date "2009-01-01" @default.
- W3090335060 modified "2023-10-02" @default.
- W3090335060 title "Spectral Energy Distributions of 6.7 GHz Methanol Masers" @default.
- W3090335060 hasPublicationYear "2009" @default.
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